Mars is cold, parched, and extremely dusty. Powerful gusts of wind kick up literal tons of reddish dust that often takes the form of whorls known as dust devils. These winds also shroud the planet in dust by lifting material from the surface and blowing it into the atmosphere (what little Mars has left of an atmosphere), sometimes creating dust storms that rage for days.
Researcher Valentin Bickel wanted to know just how intense winds can be on the red planet. Using data obtained by the Mars camera CaSSIS (Color and Stereo Surface Imaging System), the ExoMars Trace Gas Orbiter, and stereo camera HRSC (High Resolution Stereo Camera) on board ESA orbiter Mars Express, he and his team used deep learning to analyze stereo images that were taken seconds apart at the same location. These images can track the motion of dust devils, and the researchers use them to infer how the winds behind the dust devils move and lift dust from the surface. That dust goes on to have a big influence on the Martian weather.
Bickel, of the Center for Space and Habitability at the University of Bern, noticed that the tumultuous Martian winds are even faster than previous observations had made them out to be. They carry more dust than was previously thought. “Our observations show that strong near-surface winds are abundant on Mars and play an important role in atmospheric dust sourcing, directly informing more accurate models of Mars’ atmosphere, weather, and climate,” the researchers said in a study recently published in Science Advances.
